The constant magnetic field of ξ^ CMa: geometry or slow rotation?

Authors
  • C. Fourtune-Ravard
  • G.A. Wade
  • W.L.F. Marcolino
  • M. Shultz
Publication date 2011
Journal Proceedings of the International Astronomical Union
Event Active OB stars: structure, evolution, mass loss, and critical limits
Volume | Issue number 6 | S272
Pages (from-to) 180-181
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract We report recent observations of the sharp-lined magnetic βCep pulsator ξ1 CMa (= HD 46328). The longitudinal magnetic field of this star is detected consistently, but it is not observed to vary significantly, during nearly 5 years of observation. In this poster we evaluate whether the constant longitudinal field is due to intrinsically slow rotation, or rather if the stellar or magnetic geometry is responsible.
Document type Article
Note In Volume 6, S272 (July 2010) © 2011. - Part of Symposium: Active OB stars: structure, evolution, mass loss, and critical limits.
Language English
Published at
https://doi.org/10.1017/S1743921311010234 (Final published version)
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